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Search for cool extrasolar giant planets combining coronagraphy, spectral and angular differential imaging

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Academic year: 2021

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Figure 1. Left: Spectra of model atmospheres of giant planets for different effective temperatures (colored solid lines, BT-Settl models from Allard et al
Figure 2. Sensitivity limits at 5 σ of the survey in Jupiter masses of detectable companions (BT-Settl models, Allard et al

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